Introduction to Silicon Photomultiplier (Sipm)

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Introduction to Silicon Photomultiplier (Sipm) Introduction to SiPM TECHNICAL NOTE An Introduction to the Silicon Photomultiplier The Silicon Photomultiplier (SiPM) is a sensor that addresses the challenge of sensing, timing and quantifying low-light signals down to the single-photon level. Traditionally the province of the Photomultiplier Tube (PMT), the Silicon Photomultiplier now offers a highly attractive alternative that combines the low-light detection capabilities of the PMT while offering all the benefits of a solid-state sensor. The SiPM features low-voltage operation, insensitivity to magnetic fields, mechanical robustness and excellent uniformity of response. Due to these traits, the SensL SiPM has rapidly gained a proven performance in the fields of medical imaging, hazard and threat detection, biophotonics, high energy physics and LiDAR. This document provides an introduction to SiPM sensors, explaining the working principle and primary performance parameters. Contents 1. Photon Detection with SPAD and SiPM ....................................................................................................................... 2 1.1. Photon Absorption in Silicon .............................................................................................................................. 2 1.2. Silicon as a Photodiode ...................................................................................................................................... 2 1.3. The Geiger Mode in Single Photon Avalanche Diodes (SPAD) ............................................................................. 2 1.4. The Silicon Photomultiplier ................................................................................................................................. 3 1.5. SensL’s Fast Output ........................................................................................................................................... 4 1.6. Pulse Shape ....................................................................................................................................................... 4 1.7. Fill Factor ............................................................................................................................................................ 5 2. Silicon Photomultiplier Performance Parameters ........................................................................................................ 7 2.1. Breakdown Voltage and Overvoltage .................................................................................................................. 7 2.2. Gain ................................................................................................................................................................... 8 2.3. Photon Detection Efficiency and Responsivity..................................................................................................... 8 2.4. Dark Count Rate .............................................................................................................................................. 10 2.5. Optical Crosstalk .............................................................................................................................................. 11 2.6. Afterpulsing ...................................................................................................................................................... 12 2.7. Dynamic Range and Linearity ........................................................................................................................... 12 2.8. Temperature Dependency ................................................................................................................................ 13 3. Other Useful Information ............................................................................................................................................. 14 3.1. Diode Structure ................................................................................................................................................ 14 3.2. Direct Detection of Radiation with the SiPM ...................................................................................................... 14 4. Comparison with Other Sensor Technologies ............................................................................................................ 15 5. References ................................................................................................................................................................... 16 6. Further Information ...................................................................................................................................................... 16 SensL © 2011 1 Introduction to SiPM TECHNICAL NOTE 1. Photon Detection with SPAD and SiPM 1.1. Photon Absorption in Silicon When a photon travels through silicon, it may be absorbed and transfer energy to a bound electron. This absorbed energy causes the electron to move from the valence band into the conduction band, creating an electron-hole pair. The absorption depth of a photon in silicon depends on its energy (or wavelength) and is shown in Figure 1. Silicon efficiently absorbs a wide range of wavelengths of light within a depth of a few tens of microns and so is well-suited as a photodetector material. As the photon absorption is wavelength dependent, it follows that the resulting photon detection efficiency of a silicon photosensor will also be wavelength dependent. 1.2. Silicon as a Photodiode A photodiode is formed by a silicon p-n junction that creates a depletion region that is free of mobile charge carriers. When a photon is absorbed in silicon it will create an electron-hole pair. Applying a reverse bias to a photodiode sets up an electric field across the depletion region that will cause these charge carriers to Figure 1, The photon absorption depth is the depth at which be accelerated towards the anode (holes), or cathode (electrons). 1-1/e of the photons have been absorbed Therefore an absorbed photon will result in a net flow of current in a reverse-biased photodiode. 1.3. The Geiger Mode in Single Photon Avalanche Diodes (SPAD) When a sufficiently high electric field (> 5 x 105 V/cm) is generated within the depletion region of the silicon (achieved by the sensor design and application of a recommended bias), a charge carrier created there will be accelerated to a point where it carries sufficient kinetic energy to create secondary charge pairs through a process called impact ionization. In this way, a single absorbed photon can trigger a self-perpetuating ionization cascade that will spread throughout the silicon volume subjected to the electric field. The silicon will break down and become conductive, effectively amplifying the original electron-hole pair into a macroscopic current flow. This process is called Geiger discharge, in analogy to the ionization discharge observed in a Geiger- Müller tube. Vbias Figure 2, Breakdown, quench and reset cycle of Figure 3, “digital” pulse output from a a SPAD working in Geiger mode. single SPAD working in Geiger mode. SensL © 2011 2 Introduction to SiPM TECHNICAL NOTE A photodiode operated in Geiger mode employs this mechanism of breakdown to achieve a high gain and is referred to as a SPAD (Single Photon Avalanche Diode). The application of a reverse bias beyond its nominal breakdown voltage creates the necessary high-field gradients across the junction. Once a current is flowing it should then be stopped or ‘quenched’. Passive quenching (i.e. no active circuitry), is achieved through the use of a series resistor RQ which limits the current drawn by the diode during breakdown. This lowers the reverse voltage seen by the diode to a value below its breakdown voltage, thus halting the avalanche. The diode then recharges back to the bias voltage, and is available to detect subsequent photons. This cycle of breakdown, avalanche, quench and recharge of the bias to a value above the breakdown voltage, is illustrated in Figure 2. In this way, a single SPAD sensor operated in Geiger-mode functions as a photon-triggered switch, in either an ‘on’ or ‘off’ state. This results in a binary output such as illustrated in Figure 3. Regardless of the number of photons absorbed within a diode at the same time, it will produce a signal no different to that of a single photon. Proportional information on the magnitude of an instantaneous photon flux is not available. 1.4. The Silicon Photomultiplier To overcome this lack of proportionality, the Silicon Photomultiplier (SiPM) integrates a dense array of small, independent SPAD sensors, each with its own quenching resistor. Each independently operating unit of SPAD and quench resistor is referred to as a “microcell”. When a microcell in the SiPM fires in response to an absorbed photon, a Geiger avalanche is initiated causing a photocurrent to flow through the microcell. This results in a voltage drop across the quench resistor, which in turn reduces the bias across the diode to a value below the breakdown, thus quenching the photocurrent and preventing further Geiger-mode avalanches from occurring. Once the photocurrent has been quenched, the voltage across the diode recharges to the nominal bias value. The time it takes for the microcell to recharge to the full operating voltage is called the recovery time. It is important to note that the Geiger avalanche will be confined to the single microcell it was initiated in. During the avalanche process, all other microcells will remain fully
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